Astro765/CSI765


HIGH-ENERGY ASTROPHYSICS:

An Introduction to Active Galactic Nuclei



Instructor: Prof. Rita Sambruna
Time: Wednesdays, 4:30-7:10pm (Fall 2002 semester)
Place: ST1, Room 112

Unification

RATIONALE : My goal in this course is to provide you with an introduction to the physics of Active Galactic Nuclei (AGN) from an observer's perspective. What are AGN, and why are they important? What produces their tremendous power? What are the most recent developments in the study of AGN, and what are the still open questions? We will address these and other questions, and examine which tools astronomers use for their investigations of the physics of AGN.
During this course, you will familiarize yourself with up-to-date results from current and past space- and ground-based observatories, by attending the lectures, reading original scientific publications, writing essays, and participating to in-class discussions of the reading material. It is my belief that the best way to learn science is to do science. For this reason, an integral part of the course is the final hands-on project which is performed individually by the students (with my assistance). You will pick an issue that interests you, do a research project on it, and write a paper which will constitute your final. The project can be an original analysis of archival observations of AGN, or a literature search on a particular topic, or developing a theoretical idea. My objective is give you a concrete, first-hand perception of the current issues facing AGN research.

TOPICS OF LECTURES : Radiative processes in AGN; Continuum and Discrete emission; Radio, X-ray, and Gamma-ray properties; Radio-loud versus Radio-quiet AGN; Jets; Unification models; Surveys.

TEXTBOOK : The required textbook for this course is Quasars and Active Galactic Nuclei - An Introduction , by A.K.Kembhavi and J.V.Narlikar, Cambridge University Press, ISBN 0521479894.
The book will also be supplemented by papers from refereed journals. These will be used as basis for weekly discussions in class. You will need to demonstrate comprehension of the professional literature and this will count toward your final grade.

PRE-REQUISITES : Astro 530 or permission of Instructor.



  • Get a copy of the syllabus here


  • Slides of Lectures (PowerPoint):



  • Abstracts of student projects: Fall 2002

  • Useful Links for Final Project:
  • Refereed publications: ADS
    Preprints: astro/ph
    X-ray databases and other links: HEASARC
    The Chandra X-ray Observatory
    The Chandra mission
    Chandra Photo Album and Press Releases
    The XMM-Newton Observatory
    More on XMM-Newton
    Fitting engine for X-ray spectral analysis: XSPEC
    Basic information and References for sources: NED


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